Zobrazeno 1 - 10
of 92 104
pro vyhledávání: '"Stein, M A"'
Autor:
Heesen, V., Wiegert, T., Irwin, J., Crocker, R., Kiehn, A., Li, J. -T., Wang, Q. D., Stein, M., Dettmar, R. -J., Soida, M., Henriksen, R., Gajovic, L., Yang, Y., Brüggen, M.
Publikováno v:
A&A 691, A273 (2024)
Cosmic rays may be dynamically very important in driving large-scale galactic winds. Edge-on galaxies give us an outsider's view of the radio halo, which shows the presence of extra-planar cosmic-ray electrons and magnetic fields. We present a new ra
Externí odkaz:
http://arxiv.org/abs/2409.15449
Autor:
Gajović, L., Adebahr, B., Basu, A., Heesen, V., Brüggen, M., de Gasperin, F., Lara-Lopez, M. A., Oonk, J. B. R., Edler, H. W., Bomans, D. J., Paladino, R., Garduño, L. E., López-Cruz, O., Stein, M., Fritz, J., Piotrowska, J., Sinha, A.
Publikováno v:
A&A 689, A68 (2024)
Radio continuum emission from galaxies at gigahertz frequencies can be used as an extinction-free tracer of star formation. However, at frequencies of a few hundred megahertz, there is evidence for low-frequency spectral flattening. We wish to better
Externí odkaz:
http://arxiv.org/abs/2406.06689
Publikováno v:
Development of European Forests Until 2050: A Projection of Forest Resources and Forest Management in 30 Countries. :139-144
Autor:
Kadler, M., Riechers, D. A., Agarwal, J., Baczko, A. -K., Beuther, H., Bigiel, F., Birnstiel, T., Boccardi, B., Bomans, D. J., Boogaard, L., Braun, T. T., Britzen, S., Brüggen, M., Brunthaler, A., Caselli, P., Elsässer, D., von Fellenberg, S., Flock, M., Fromm, C. M., Fuhrmann, L., Hartogh, P., Hoeft, M., Keenan, R. P., Kovalev, Y., Kreckel, K., Livingston, J., Lobanov, A. P., Müller, H., Ros, E., Schilke, P., De Simone, M., Spitler, L., Ueda, T., Vardoulaki, E., Vegetti, S., Weis, K., Wendel, C., Xu, M. H., Zhao, G. -Y., Albrecht, M., Basu, A., Tjus, J. Becker, Bernhart, S., Blum, J., Bonnassieux, E., Bredendiek, C., van Delden, M., Di Gennaro, G., Enders, A., Eppel, F., Hase, H., Hoang, D., Hugentobler, U., Kaasinen, M., Krupp, N., Kun, E., Laubach, M., Lin, Y., Mannheim, K., Menten, K. M., Perkuhn, R., Pohl, N., Powell, D. M., Rezzolla, L., Ricci, L., Schinnerer, E., Schmidt, K., Schöpfel, J., Stanko, S., Stein, M., Sulzenauer, N., Taziaux, S., Tursunov, A., Walter, F., Weiss, A., Witzel, G., Wolf, S., Zensus, J. A., Mus, A., Toth, L. V., Alberdi, A., Benisty, M., Cox, P., Guirado, J. C., Johnson, M. D., Juvela, M., Neeleman, M., Pashchenko, I. N., Torres, M. A. Pérez, Perraut, K., Zajacek, M.
The Next Generation Very Large Array (ngVLA) is a planned radio interferometer providing unprecedented sensitivity at wavelengths between 21 cm and 3 mm. Its 263 antenna element array will be spatially distributed across North America to enable both
Externí odkaz:
http://arxiv.org/abs/2311.10056
Autor:
Heesen, V., Schulz, S., Brüggen, M., Edler, H., Stein, M., Paladino, R., Boselli, A., Ignesti, A., Fossati, M., Dettmar, R. -J.
Context. In order to understand galaxy evolution, it is essential to measure star formation rates (SFRs) across Cosmic times. Aims. The use of radio continuum emission as an extinction-free star formation tracer necessitates a good understanding of t
Externí odkaz:
http://arxiv.org/abs/2309.05732
Akademický článek
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Autor:
Heesen, V., O'Sullivan, S. P., Brüggen, M., Basu, A., Beck, R., Seta, A., Carretti, E., Krause, M. G. H., Haverkorn, M., Hutschenreuter, S., Bracco, A., Stein, M., Bomans, D. J., Dettmar, R. -J., Chyży, K. T., Heald, G. H., Paladino, R., Horellou, C.
Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely unconstrained. Their detection is important as magnetic fields can have a significant impact on the evolution of the CGM and, in turn, the fields can serve as tra
Externí odkaz:
http://arxiv.org/abs/2302.06617
Autor:
Heesen, V., de Gasperin, F., Schulz, S., Basu, A., Beck, R., Brüggen, M., Dettmar, R. -J., Stein, M., Gajović, L., Tabatabaei, F. S., Reichherzer, P.
Publikováno v:
A&A 672, A21 (2023)
Context. The details of cosmic-ray transport have a strong impact on galaxy evolution. The peak of the cosmic-ray energy distribution is observable in the radio continuum using the electrons as proxy. Aims. We measure the length that the cosmic-ray e
Externí odkaz:
http://arxiv.org/abs/2212.06585
Autor:
Stein, M., Heesen, V., Dettmar, R. -J., Stein, Y., Brüggen, M., Beck, R., Adebahr, B., Wiegert, T., Vargas, C. J., Bomans, D. J., Li, J., English, J., Chyzy, K. T., Paladino, R., Tabatabaei, F. S., Strong, A.
Publikováno v:
A&A 670, A158 (2023)
Galactic winds play a key role in regulating the evolution of galaxies over cosmic time. In recent years, the role of cosmic rays (CR) in the formation of the galactic wind has increasingly gained attention. Therefore, we use radio continuum data to
Externí odkaz:
http://arxiv.org/abs/2210.07709
Autor:
Heesen, V., Klocke, T. -L., Brüggen, M., Tabatabaei, F. S., Basu, A., Beck, R., Drabent, A., Nikiel-Wroczyński, B., Paladino, R., Schulz, S., Stein, M.
Publikováno v:
A&A 669, A8 (2023)
Context. Magnetic fields are key to understand galaxy evolution, regulating stellar feedback and star formation in galaxies. Aims. We probe the origin of magnetic fields in late-type galaxies, measuring magnetic field strengths, exploring whether mag
Externí odkaz:
http://arxiv.org/abs/2208.11068